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(65407) 2002 RP120
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Trans-Neptunian object
August 2026
yes
(65407) 2002 RP 120
#C2E0FF
LONEOS
Anderson Mesa Stn.
4 September 2002
(65407) 2002 RP 120
TNOdamocloidunusualdistant
27 April 2019 (JD 2458600.5)
2
3.35 yr (1,225 d)
105.39 AU
2.4544 AU
53.920 AU
0.9545
395.95 yr (144,619 d)
15.061°
0.0025 ms / day
118.97°
39.263°
357.79°
−0.8340
14.6 2.8 km
200 h
0.098 0.036
B–R 1.37
12.3
(65407) 2002 RP 120 is a trans-Neptunian object and damocloid from the outer Solar System. Its orbit is retrograde and comet-like, and has a high eccentricity. It was discovered on 4 September 2002 by astronomers with the LONEOS survey at Anderson Mesa Station, Arizona, in the United States. The unusual object measures approximately 14.6 km mi off us in diameter and is likely elongated in shape. It is a slow rotator and potentially a tumbler as well. The object was probably ejected from the ecliptic by Neptune.November 2018
Orbit and classification
2002 RP 120 is a member of the damocloids, with a retrograde orbit and a negative TJupiter of −0.8340. It is also a trans-Neptunian object, as its orbit has a semi-major axis larger than that of Neptune (30.1 AU). The Minor Planet Center lists it as a critical object, centaur, and (other) unusual minor planet due to an orbital eccentricity of more than 0.5.
It orbits the Sun at a distance of 2.5–105 AU once every 396 years (semi-major axis of 53.92 AU). Its orbit has an eccentricity of 0.95 and an inclination of 119° with respect to the ecliptic. The body's observation arc begins with a precovery taken by Astrovirtel I03 at ESO's La Silla Observatory in February 2001, or 19 months prior to its official discovery observation at Anderson Mesa.
Numbering and naming
This minor planet was permanently numbered 65407 (65407) by the Minor Planet Center on 14 June 2003 (M.P.C. 48994). As of 2018, it has not been named.
Physical characteristics
The object has a B–R magnitude of 1.37, typical for most dynamical groups in the outer Solar System.
Rotation period
In October 2010, a rotational lightcurve of 2002 RP 120 was obtained from photometric observations by French amateur astronomer René Roy. Lightcurve analysis gave a rotation period of 200 hours with a brightness amplitude of 0.6 magnitude, indicative of an elongated, non-spherical shape (U=2). With a rotation period above 100 hours, it is a typical slow rotator.
Diameter and albedo
According to the survey of minor-planet albedos of bodies in a comet-like orbit, carried out by Yanga Fernández in collaboration with David Jewitt and Scott Sheppard at the Institute for Astronomy, Hawaii, 2002 RP 120 measures 14.6 kilometers in diameter and its surface has an albedo of 0.098. Johnston's archive gives a rounded figure of 15 kilometers.
References
2004-06-22 last obs.
JPL Small-Body Database Browser: 65407 (2002 RP120)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2065407
Jet Propulsion Laboratory
20 November 2018
65407 (2002 RP120)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=65407
20 November 2018
MPC/MPO/MPS Archive
Minor Planet Center
https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html
20 November 2018
List of Other Unusual Objects
Minor Planet Center
14 November 2018
https://www.minorplanetcenter.net/iau/lists/t_others.html
20 November 2018
List of Known Trans-Neptunian Objects
Johnston's Archive
30 December 2017
Johnston Wm. Robert
http://www.johnstonsarchive.net/astro/tnoslist.html
1 March 2018
Asteroids and comets rotation curves – (65407)
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page5cou.html#065407
1 March 2018
https://web.archive.org/web/20181111134209/http://obswww.unige.ch/~behrend/page5cou.html#065407
11 November 2018
dead
65407
1 March 2018
Yanga R. Fernández
David C. Jewitt
Scott S. Sheppard
July 2005
Albedos of Asteroids in Comet-Like Orbits
The Astronomical Journal
130
1
308–318
2005AJ....130..308F
10.1086/430802
53642261
External links
List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
(65407) 2002 RP120 https://web.archive.org/web/20200915150345/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=65407 15 September 2020 , Small Bodies Data Ferret
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Category:Minor planets with a retrograde orbit
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